Recent cosmological observations have shown that our universe is experiencing a late-time acceleration [1]}, [2]}.
The simplest attempt to explain this phenomenon is to introduce the cosmological constant
\(\Lambda \)  as a repulsive force effectively, which is also embedded in the \(\Lambda \) CDM model [3]}, [4]}.
Although the \(\Lambda \) CDM model is one of the most successful cosmological model describing the large-scale structure of the universe,
it fails to solve the fine-tuning and
coincidence problems, referred to as the cosmological constant problem [5]}, [6]}, [7]}.
